Automated reconstruction of subsurface interfaces in Promethei Lingula near the Martian south pole by using SHARAD data

Subsurface layers are preserved in polar regions on Mars, which are considered to be a record of past climate changes on Mars. Orbital radar instruments like the SHAllow RADar (SHARAD) on board Mars Reconnaissance Orbiter (MRO) transmit radar signals to Mars and receive a set of signals returned fro...

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Bibliographic Details
Main Authors: Xiong, S, Muller, JP
Format: Article in Journal/Newspaper
Language:English
Published: 2018
Subjects:
Online Access:https://discovery.ucl.ac.uk/id/eprint/10055510/1/Xiong_Automated.pdf
https://discovery.ucl.ac.uk/id/eprint/10055510/
id ftucl:oai:eprints.ucl.ac.uk.OAI2:10055510
record_format openpolar
spelling ftucl:oai:eprints.ucl.ac.uk.OAI2:10055510 2023-12-24T10:24:53+01:00 Automated reconstruction of subsurface interfaces in Promethei Lingula near the Martian south pole by using SHARAD data Xiong, S Muller, JP 2018-01-01 text https://discovery.ucl.ac.uk/id/eprint/10055510/1/Xiong_Automated.pdf https://discovery.ucl.ac.uk/id/eprint/10055510/ eng eng https://discovery.ucl.ac.uk/id/eprint/10055510/1/Xiong_Automated.pdf https://discovery.ucl.ac.uk/id/eprint/10055510/ open Planetary and Space Science (2018) (In press). Martian south pole Subsurface mapping Radar stratigraphy Promethei Lingula SHARAD Article 2018 ftucl 2023-11-27T13:07:39Z Subsurface layers are preserved in polar regions on Mars, which are considered to be a record of past climate changes on Mars. Orbital radar instruments like the SHAllow RADar (SHARAD) on board Mars Reconnaissance Orbiter (MRO) transmit radar signals to Mars and receive a set of signals returned from interfaces having a contrast in dielectric properties in the probed subsurface regions. These subsurface layers which are preserved in the upper ≈ 1 km of the Martian Polar Layered Deposits (PLDs) can be observed in SHARAD radargrams. Extraction of these layering features is the preliminary work before interpreting and understanding their origins. In this study, we use a new method based on log-Gabor filtering and Continuous Wavelet Transform (CWT)-based peak detection to extract subsurface radar reflections and a workflow to remove clutter reflections in order to reconstruct 3-D subsurface layers. These methods and workflow are then tested on the SHARAD data in the Promethei Lingula region near the Martian south pole. The results show that following this workflow, the ground surface and six subsurface interfaces can be reconstructed, which aids in the interpretation of the depositional and erosional history of this region. Article in Journal/Newspaper South pole University College London: UCL Discovery South Pole
institution Open Polar
collection University College London: UCL Discovery
op_collection_id ftucl
language English
topic Martian south pole
Subsurface mapping
Radar stratigraphy
Promethei Lingula
SHARAD
spellingShingle Martian south pole
Subsurface mapping
Radar stratigraphy
Promethei Lingula
SHARAD
Xiong, S
Muller, JP
Automated reconstruction of subsurface interfaces in Promethei Lingula near the Martian south pole by using SHARAD data
topic_facet Martian south pole
Subsurface mapping
Radar stratigraphy
Promethei Lingula
SHARAD
description Subsurface layers are preserved in polar regions on Mars, which are considered to be a record of past climate changes on Mars. Orbital radar instruments like the SHAllow RADar (SHARAD) on board Mars Reconnaissance Orbiter (MRO) transmit radar signals to Mars and receive a set of signals returned from interfaces having a contrast in dielectric properties in the probed subsurface regions. These subsurface layers which are preserved in the upper ≈ 1 km of the Martian Polar Layered Deposits (PLDs) can be observed in SHARAD radargrams. Extraction of these layering features is the preliminary work before interpreting and understanding their origins. In this study, we use a new method based on log-Gabor filtering and Continuous Wavelet Transform (CWT)-based peak detection to extract subsurface radar reflections and a workflow to remove clutter reflections in order to reconstruct 3-D subsurface layers. These methods and workflow are then tested on the SHARAD data in the Promethei Lingula region near the Martian south pole. The results show that following this workflow, the ground surface and six subsurface interfaces can be reconstructed, which aids in the interpretation of the depositional and erosional history of this region.
format Article in Journal/Newspaper
author Xiong, S
Muller, JP
author_facet Xiong, S
Muller, JP
author_sort Xiong, S
title Automated reconstruction of subsurface interfaces in Promethei Lingula near the Martian south pole by using SHARAD data
title_short Automated reconstruction of subsurface interfaces in Promethei Lingula near the Martian south pole by using SHARAD data
title_full Automated reconstruction of subsurface interfaces in Promethei Lingula near the Martian south pole by using SHARAD data
title_fullStr Automated reconstruction of subsurface interfaces in Promethei Lingula near the Martian south pole by using SHARAD data
title_full_unstemmed Automated reconstruction of subsurface interfaces in Promethei Lingula near the Martian south pole by using SHARAD data
title_sort automated reconstruction of subsurface interfaces in promethei lingula near the martian south pole by using sharad data
publishDate 2018
url https://discovery.ucl.ac.uk/id/eprint/10055510/1/Xiong_Automated.pdf
https://discovery.ucl.ac.uk/id/eprint/10055510/
geographic South Pole
geographic_facet South Pole
genre South pole
genre_facet South pole
op_source Planetary and Space Science (2018) (In press).
op_relation https://discovery.ucl.ac.uk/id/eprint/10055510/1/Xiong_Automated.pdf
https://discovery.ucl.ac.uk/id/eprint/10055510/
op_rights open
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